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Non-Geometric String Theory Backgrounds from Gauged Supergravities to Interacting Chiral Bosons ≺
Nikolaos Prezas
Albert Einstein Center for Fundamental PhysicsInstitute for Theoretical Physics
University of Bern
based on• "Conformal Chiral Boson Models on Twisted Doubled Tori and Non-Geometric
String Backgrounds", with S. Avramis and J. P. Derendinger,Nucl. Phys. B827 (2010) 281; arXiv:0910.0431
• "Worldsheet Theories for Non-Geometric String Backgrounds",with G. Dall’Agata, JHEP 0808 (2008) 088; arXiv:0712.1026
• "Gauged Supergravities from Twisted Doubled Tori and Non-Geometric StringBackgrounds", with G. Dall’Agata, H. Samtleben and M. Trigiante,Nucl. Phys. B799 (2008) 80; arXiv:0712.1026
Motivation and overview
Fluxes, twists and supergravity gaugings
Non-geometric backgrounds and twisted doubled tori
Interacting chiral boson models: Lorentz invariance
Interacting chiral boson models: one-loop effective action
Summary and open problems
Standard lore about string theory
I Consistent unification of gauge and gravitational interactions• However, it requires (typically) more dimensions than four!• How can we make contact to four-dimensional physics ?
Compactification approach
I Assumption: spacetime of the formM4 × Y6
• Classify possible internal spaces Y6
• Derive effective theory in 4 dimensions
Traditional compactification scheme (80s)
I Non-trivial metric on Y6 + SUSY → Calabi–Yau(or manifolds with exceptional holonomy)• However: huge vacuum degeneracy• Moduli: scalars without potential (fluctuations of internal
fields)• Problems: long range forces + loss of predictive power• Moduli stabilization
Flux compactifications (90s)
I Enlarge landscape: fluxes of antisymmetric tensor fieldsI Generate potential for "moduli" fields• Special holonomy → manifolds with G -structure• Scalar potential + extended SUSY: gauged supergravity• Fluxes ↔ gauging parameters
Scherk–Schwarz reductions - twisted tori - geometric fluxes
I Twisted reduction on a torus: twisted torus[Scherk, Schwarz ’79; Kaloper, Myers ’99]
• Induces scalar potential and non-abelian gauge symmetry• Consistent truncation on a (local) group manifold
Are there more general backgrounds/fluxes ?
I Non-geometric backgrounds: T-folds[Flournoy, Wecht, Williams ’02; Hellerman, McGreevy, Williams ’02; Dabholkar, Hull ’02;
Kachru, Schulz, Tripathy, Trivedi ’02]
• Background data: patched with T-dualities• Associated non-geometric fluxes (from duality covariance)
[Shelton, Taylor, Wecht ’05; Dabholkar, Hull ’05; Aldazabal, Camara, Font, Ibanez ’06; Shelton,
Taylor, Wecht ’06]
Are there more general effective theories ?
I General framework: embedding tensor[de Wit, Samtleben, Trigiante ’05]
• Yields all supergravity gaugings for N ≥ 1
Non-geometric backgrounds and doubled geometries
I Inherently stringy constructions: winding modes• Doubling of coordinates
[Witten ’88; Duff ’90; Tseytlin ’90, ’91; Kugo, Zwiebach ’92; Maharana, Schwarz ’92; Siegel ’93]
• Doubled torus: geometry for non-geometric string backgrounds[Hull ’04, ’06, ’07]
• Twisted doubled torus (TDT): electric N = 4 gaugings[Hull, Reid-Edwards ’07; Dall’Agata, Prezas, Samtleben, Trigiante ’07]
Worldsheet approach: chiral bosons
I Momentum and winding modes on equal footing: chiral bosons[Siegel ’84; Floreanini, Jackiw ’87]
• Interacting models: conditions from 2d Lorentz invariance[Tseytlin ’90, ’91]
• TDT as target space: Lorentz invariant![Dall’Agata, Prezas ’08]
• Conditions for conformal invariance[Avramis, Derendinger, Prezas ’09]
• Computation of the one-loop effective action• Agreement with corresponding gauged supegravity
Motivation and overview
Fluxes, twists and supergravity gaugings
Non-geometric backgrounds and twisted doubled tori
Interacting chiral boson models: Lorentz invariance
Interacting chiral boson models: one-loop effective action
Summary and open problems
Compactifications without fluxes
I Consider a toroidal reduction of string/M-theory• Abelian gauge theory without scalar potential• Existence of global duality symmetries
[Cremmer, Scherk, Ferrara ’79; Cremmer, Julia ’79]
Flux compactifications
I Our setup: heterotic strings on T6 (ignoring the gauge sector)I Let us assume NS-NS 3-form flux in the internal torus:
〈Hijk(x , y)〉 = hijk
• Decompose 2-form, metric tensor and dilaton:
BMN(x , y) → Bµν(x),Bµi (x),Bij (x)GMN(x , y) → Gµν(x),Gµi (x),Gij (x)
φ(x , y) → φ(x)
• 3-form kinetic term yields potential for metric moduli∫M4×T6
H ∧∗H =∫M4
d4x√−g4(hijkhmlnG im(x)G jl (x)G kn(x)+ · · · )
and non-abelian gauge interactions∫M4
d4x√−g4(· · ·+ ∂µB i
νGµjG νkhijk + · · · )
• Generators: Zi for Gµi , X i for Bµi . Gauge algebra:
[X i ,X i ] = 0[Zi ,X j ] = 0[Zi ,Zj ] = hijkX k
Scherk-Schwarz reductions (a.k.a. twisted tori, geometric fluxes)
I Can we enrich the previous gauge algebra ?I Consider reduction ansatz
ds2(10) = Gµν(x)dxµdxν
+ (δab + Gab(x))(ηa + Aaµ(x)dx
µ)(ηb + Abν(x)dx
ν)
with ηa(y) being left-invariant 1-forms satisfying
dηa = −12
τ abc ηb ∧ ηc
• Similar expansion for other fields• τ a
bc are structure constants of Lie algebra g (Jacobi identity)I Consistent truncation to singlets under GL
[Duff, Pope ’85; Hull, Reid-Edwards ’05]
I Geometric flux: spin connection condensate
〈ω abc (x , y)〉 = 1
2τ abc
• Compactification on a twisted torus: local group manifold G/ΓI Equivalent to a twisted reduction on a torus
[Scherk, Schwarz ’79]
ηa(y) = Uaj (y)dy
i
• Introduces y -dependance that is eliminated if
U−1ib (y)U−1j
c (y)∂[iUaj ] = τ a
bc
I Combining with NS-NS flux yields gauge algebra:[Kaloper, Myers ’99]
[X a,X b] = 0[X a,Zb] = τ a
bc X c
[Za,Zb] = τ cab Zc + habcX c
• Part of isometry group GR appears as gauge symmetry
• Introduce XA = Za,X a, gauge algebra:
[XA,XB ] = TABCXC
• Fluxes ⇒ gauge algebra structure constants TABC
• Jacobi for TABC : Bianchi for fluxes and Jacobi for τ abc
I Pack scalar fields in O(6,6)O(6)×O(6) matrix:
MAB =
(Gab − BacG cdBdb BacG cb
−GbcBca G ab
)• Scalar potential:
V ∼ T CDA T D
CB MAB +13T ACE T B
DF MABMCDMEF
I What type of theory is this ?• 4 dimensions, 16 supersymmetries, gravity, non-abelian gauge
symmetry, scalar potential =⇒ N = 4,D = 4 gaugedsupergravity[Kaloper, Myers ’99]
General gauge algebras[Shelton, Taylor, Wecht ’05; Dabholkar, Hull ’05; Aldazabal, Camara, Font, Ibanez ’06]
I Fill in the gaps in Kaloper–Myers gauge algebra:
[Za,Zb] = τ cab Zc + habcX c
[X a,Zb] = τ abc X c −Q ac
b Zc[X a,X b] = Q ab
c X c + RabcZc
• Physical and geometric fluxes: non-semisimple gauge groups• Q ab
c : non-abelian gauge symmetry from B-field gauge vectors!I What is the origin of the new "fluxes" Q and R ? T-dualityI Organizing principle: N = 4,D = 4 gauged supergravity
Gauged supergravity perspective
I General gauging: adjoint of gauge group → fundamental ofduality group[de Wit, Samtleben, Trigiante ’05]
XA = θmA tm
• Embedding tensor θaM : subject to conditions ⇒ full theory• In particular: gauge algebra ⇒ all possible fluxes!
I Focus on N = 4,D = 4 gauged supergravity• N = 4 graviton multiplet: graviton, axio-dilaton, 6 vectors• N = 4 vector multiplet: vector, 6 scalars• Duality group of ungauged theory: SL(2)×O(6, 6+ n)• Scalars
τ ∈ SL(2)U(1)
, MAB ∈O(6, 6+ n)
O(6)×O(6+ n)
• Embedding tensor (subject to quadratic constraints)[Schön, Weidner ’06]
fαABC , ξαA
• Heterotic reduction (n = 0): T-duality group O(d , d), d = 6
• Electric gaugings
f−ABC = 0, ξαA = 0
• For electric gaugings: embedding tensor ≡ structure constants
f+ABC := fABC = TABDηCD = TABC
• O(d , d) metric ηAB
ηAB =
(0 1d
1d 0
)• N = 4 gauge algebra
[XA,XB ] = TABCXC
• ηAB invariant metric on gauge algebra• N = 4 scalar potential
V (M) ∼ 12
(13MAA′MBB ′MCC ′ +
(23
ηAA′ −MAA′)
ηBB ′ηCC ′)TABCTA′B ′C ′
• Consider geometric T6 symmetry: GL(6) ⊂ O(6, 6)I Decompose fundamental rep 12→ 6⊕ 6
XA = Za,X a
fABC = (fabc , f cab , f bc
a , f abc)
• N = 4 electric gaugings: include all possible (NS-NS) fluxes[Derendinger, Petropoulos, Prezas ’07]
habc , τ cab ,Q bc
a ,Rabc
• There is a similar set of S-dual fluxes: f−ABC• ξαI : reduction with SO(1, 1) duality twist
[Derendinger, Petropoulos, Prezas ’07]
I Similar story: N = 8 gauged supergravity (type II/M-theory )
Motivation and overview
Fluxes, twists and supergravity gaugings
Non-geometric backgrounds and twisted doubled tori
Interacting chiral boson models: Lorentz invariance
Interacting chiral boson models: one-loop effective action
Summary and open problems
Duality related backgrounds
I h, τ,Q,R are related by T-dualityI Toy model (not a solution but can be promoted to one)
[Kachru, Schulz, Tripathy, Trivedi ’02; Lowe, Nastase, Ramgoolam ’03]
• 3-torus with N units of NS-NS flux hxyz
ds2 = dx2 +dy2 +dz2, H = Ndx ∧dy ∧dz , B = Nxdy ∧dz
• x ∼ x + 1: gauge transformation on BI T-duality along z ⇒ twisted torus (geometric flux τz
xy )
ds2 = dx2 + dy2 + (dz +Nxdy)2, H = 0
τy ,z (x) = Nx + i
• x ∼ x + 1: SL(2;Z) modular transformation on fiber T2y ,z
• Bianchi II or nilmanifold
I T-duality along y ⇒ T-fold (Q-flux Qzyx )
ds2 = dx2 +1
1+N2x2 (dz2 + dy2), B =
Nx1+N2x2 dy ∧ dz
• x ∼ x + 1: T-duality group O(2, 2;Z) action onMAB ≡ Gab,Bab
MAB(x + 1) =
1 0 0 00 1 0 00 −N 1 0N 0 0 1
MAB(x)
• There is a local geometric description• Globally well-defined up to T-duality• In this sense: non-geometric
I T-duality along x : cannot be done using Buscher rules• At the level of the effective theory: R-flux Rxyz
• In this case there is no local geometric description• Explicit dependance on dual coordinate xI Other non-geometric string constructions: S-folds, U-folds,
mirror-folds, asymmetric orbifolds, CFT constructions
Doubling and doubled tori[Witten ’88; Duff ’90; Tseytlin ’90, ’91; Kugo, Zwiebach ’92; Maharana, Schwarz ’92]
I y i conjugate to momenta, y i conjugate to windings• Double coordinates Y I = y i , y i ⇒ doubled torus T2n
dS2 = 2dy idyi , O(n, n;Z) ∈ GL(2n;Z)
• Realize T-duality group O(n, n;Z) geometricallyI Geometry for non-geometric string backgrounds
[Hull ’04, ’06, ’07]
I Scherk–Schwarz: torus → twisted torus → geometric fluxesI Natural idea: why not double everything and then twist• Generalization of Scherk–Schwarz on the doubled torus!
Twisted doubled tori (TDT)[Hull, Reid-Edwards ’07; Dall’Agata, Prezas, Samtleben, Trigiante ’07]
I Consider ordinary compactification on Td
• Full gauge group U(1)2d : isometry of the doubled torus T2d
• Suggests: generic gauging G from twisting the doubled torus!• Generalization of Scherk–Schwarz via a double field theoryI Gauge algebra and Gab potential in Scherk-Schwarz reduction
(twisted torus) of pure gravity:
[Za,Zb] = τkabZc
V ∼ 2 τabc τb
ad gcd + τa
bc τdef gadg
beg cf
• Gauge algebra XA = Za,X a and MAB ≡ Gab,Babpotential for electric N = 4 gaugings (twisted doubled torus)
[XA,XB ] = TABCXC
V ∼ 3 T CDA T D
CB MAB + T ACE T B
DF MABMCDMEF
• MAB "metric" moduli on twisted doubled torus
I General gauging: Scherk–Schwarz – but doubled!I Geometric flux on doubled torus ⇔ all fluxesI Twisted doubled torus (TDT): local group manifold G
EA = EAI (Y )dY I
dEA = −12T ABCE
B ∧ EC
T ABC = habc , τ a
bc ,Q bca ,Rabc
I Geometric interpretation of embedding tensorI Gauging ⇔ Fluxes ⇔ TDT =⇒ spacetime data (partially)
[Dall’Agata, Prezas, Samtleben, Trigiante ’07]
I Is it really the underlying geometry or just bookkeeping tool ?
Motivation and overview
Fluxes, twists and supergravity gaugings
Non-geometric backgrounds and twisted doubled tori
Interacting chiral boson models: Lorentz invariance
Interacting chiral boson models: one-loop effective action
Summary and open problems
Chiral bosons
I Twisted doubled torus as string target space ?• Treat momentum and winding independentlyI Chiral boson theory
[Siegel ’84; Floreanini, Jackiw ’87]
• Floreanini–Jackiw (FJ) approach (∂± = ∂0 ± ∂1)
S+ =12
∫d2σ∂1φ+∂−φ+
∂1(∂−φ+) = 0⇒ ∂−φ+ = 0
• Lorentz invariant on-shell
δLS+ =12
∫d2σ(∂−φ+)
2
• Similarly for antichiral boson S− = − 12
∫d2σ∂1φ−∂+φ−
I Introducing usual and dual fields
φ =1√2(φ+ + φ−), χ =
1√2(φ+ − φ−)
S = S++S− =12
∫d2σ
(∂0φ∂1χ+ ∂1φ∂0χ− (∂1φ)2− (∂1χ)2
)• Symmetric under φ↔ χ
• Double integration by parts, set p = ∂1χ: first order
S =12
∫d2σ
(2∂0φp − (∂1φ)2 − p2
)• Non-local duality relation p ≡ ∂1χ = ∂0φ
• Second order action of free boson φ
S =12
∫d2σ
((∂0φ)2 − (∂1φ)2
)
I T-duality invariant formulation• Start with compact boson at radius R
S =R2
2
∫d2σ
((∂0φ)2 − (∂1φ)2
)• First order
S =12
∫d2σ
(− p2
R2 + 2p∂0φ− (R∂1φ)2)
• Introduce dual field ∂1χ = p, integrate by parts
S =12
∫d2σ
(∂1χ∂0φ + ∂0χ∂1φ− (R−1∂1χ)2 − (R∂1φ)2
)• Manifest T-duality invariance: φ↔ χ,R ↔ R−1
• Dual boson at radius R−1
S =R−2
2
∫d2σ
((∂0χ)2 − (∂1χ)2
)
Interacting chiral bosons
I Consider the following action (YI = y i , y i)[Tseytlin ’90, ’91]
S =12
∫d2σ
(−HIJ (Y)∂1YI ∂1YJ +
(ηIJ (Y) + CIJ (Y)
)∂0YI ∂1YJ
)• HIJ , ηIJ : symmetric, CIJ antisymmetric• Interacting generalization of Floreanini-JackiwI Free theory
HIJ =
(1d 00 1d
), ηIJ =
(0 1d
1d 0
), CIJ = const.
• Yields d + d copies of FJ for y i± = y i ± y i : double torus• Integrate out y i (or y i ): original (or dual) torus vacuum
I Lorentz invariance condition
ηIJ
(∂0YI ∂0YJ + ∂1YI ∂1YJ
)− 2HIJ∂0YI ∂1YJ = 0
• Rearrange to(η −Hη−1H
)IJ ∂1YI ∂1YJ + ηIJVIVJ = 0 with
VI ≡ ηIJ∂0YJ −HIJ∂1YJ
• Sufficient (η −Hη−1H
)IJ = 0 and ηIJVIVJ = 0
• Notice: equation of motion
2∂1VI + ∂IHJK ∂1YJ∂1YK
− GIJK ∂0YJ∂1YK − 2ηJLΓLIK (η)∂0YJ∂1YK = 0
I Lorentz invariant modelsI Standard sigma models
[Tseytlin ’90, ’91]
HIJ =
(Gij − BikGklBlj BikGkj
−G ikBkj G ij
), ηIJ =
(0 1d
1d 0
),CIJ = const.
• Metric Gij = Gij (y), B-field Bij = Bij (y)• Integrating out y i
S =∫
d2σ(√
γγµνGij + εµνBij )∂µy i∂νy j
I Interacting non-abelian chiral scalars[Depireux, Gates, Park ’89; Gates, Siegel ’88; Tseytlin ’90, ’91]
I η = ±H: quantum Lorentz anomaly[Dall’Agata, Prezas ’08]
I Twisted doubled tori[Dall’Agata, Prezas ’08]
• Gauge algebra → group representative → vielbein
dEA = −12T ABCE
B ∧ EC , EA = EAI (Y )dY I
• Construct ηIJ and HIJ as
ηIJ = ηABEAI E
BJ ; ηAB =
(0 1d
1d 0
)HIJ = HABEA
I EBJ ; ηAB = HACηCDHDB
• HAB ∈ O(d ,d)O(d)×O(d) (cf. N = 4 moduli MAB)
• First Lorentz invariance condition is satisfied by construction• Add generalized three-form flux
GABC = 3∂[ACBC ] = TABC
• Equation of motion reads
(DIVJ −12T KIJ VK )∂1YI = 0
• Second Lorentz invariance condition is satisfied• Compact gaugings
TABDHDC = −TACDHDB
• Choose GABC = −TABC ⇒ V I = 0• Electric N = 4 gauging and moduli matrix MAB ⇔
Lorentz invariant chiral boson model• Related (equivalent ?) second order constrained formulation
[Albertsson, Kimura, Reid-Edwards ’08, Hull, Reid-Edwards ’09, Reid-Edwards ’09]
I Application: recover spacetime background fields[Dall’Agata, Prezas ’08]
• Impossible to integrate out dual coordinates for R-flux• No local geometric description
Motivation and overview
Fluxes, twists and supergravity gaugings
Non-geometric backgrounds and twisted doubled tori
Interacting chiral boson models: Lorentz invariance
Interacting chiral boson models: one-loop effective action
Summary and open problems
One-loop effective action
I Can the TDT models be promoted to conformal field theories ?I Starting point
S =12
∫d2σ
(−HIJ (Y)∂1YI ∂1YJ +
(ηIJ (Y) + CIJ (Y)
)∂0YI ∂1YJ
)• Earlier work: HIJ and ηIJ depend on base coordinates Xm
[Berman, Copland, Thompson ’07; Berman, Copland ’07]
• Background field method YI = YIcl + πI (ξI )
[Alvarez-Gaume, Freedman, Mukhi ’81; Braaten, Curtright, Zachos ’85; Mukhi ’86; Howe,
Papadopoulos, Stelle ’88]
• Covariant expansion, recursive algorithm[Mukhi ’86]
Sn =1n!DnS ≡ 1
n!
(∫d2σξI (σ)
DDYI (σ)
)n
S
I η-covariant expansion
S1 =∫
d2σ( 1
2ηIJ (∂0YID1ξJ +D0ξI ∂1YJ )−HIJ∂1YID1ξJ
− 12DKHIJ ξK ∂1YI ∂1YJ +
12GIJK ξK ∂0YI ∂1YJ
)
S2 =12
∫d2σ
(−HIJD1ξID1ξJ + ηIJD0ξID1ξJ
+
(12DJGIKL + RKIJL
)ξI ξJ∂0YK ∂1YL
− 12(DIDJHKL +HKMRM
IJL +HLMRMIJK )ξI ξJ∂1YK ∂1YL
+12GIJK ξK (∂0YID1ξJ +D0ξI ∂1YJ )− 2DKHIJξKD1ξI ∂1YJ
)
I One-loop effective action Seff = Scl + Γ
exp (iΓ[Y]) =∫Dξ exp (iS2[Y; ξ])
I Propagators of tangent space fields ξA
[Tseytlin ’90, ’91; Berman, Copland, Thompson ’07]
〈ξA(σ)ξB(σ′)〉 = HAB∆(σ− σ′) + ηAB ∆(σ− σ′)
∆(σ− σ′) =12(∆+(σ− σ′) + ∆−(σ− σ′)
)= − 1
4πln(σ− σ′)2
∆(σ− σ′) =12(∆+(σ− σ′)− ∆−(σ− σ′)
)= − 1
2πarctanh
σ1 − σ′1
σ0 − σ′0
• Regularize: ln(σ− σ′)2 → ln((σ− σ′)2 + µ2), set
σ1−σ′1
σ0−σ′0 = tanh δ
• Limiting expressions
∆(0)→ − 12π
ln µ , ∆(0)→ − 12π
δ
• Breakdown of scale invariance and Lorentz invariance
I Weyl anomaly and global Lorentz anomaly
W =12
∫d2σ
(W 00
IJ ∂0YI ∂0YJ +W 01IJ ∂0YI ∂1YJ +W 11
IJ ∂1YI ∂1YJ)
L =12
∫d2σ
(L00IJ ∂0YI ∂0YJ + L01IJ ∂0YI ∂1YJ + L11IJ ∂1YI ∂1YJ
)• Vanishing on-shell: equations of motion and/or constraints• Weyl anomaly coefficients:
W 00IJ =
14(HA[CHD]B − ηA[C ηD]B )Q0
AB,IQ0CD,J
W 01IJ = HABS01AB,IJ +
12(HA[CHD]B − ηA[C ηD]B )Q0
AB,IQ1CD,J
− 14(HA[C ηD]B + ηA[CHD]B )
(Q0
AB,IP1CD,J + P1
AB,IQ0CD,J
)W 11
IJ = HABS11AB,IJ +14(HA[CHD]B − ηA[C ηD]B )Q1
AB,IQ1CD,J
− 14(HA[C ηD]B + ηA[CHD]B )
(Q1
AB,IP1CD,J + P1
AB,IQ1CD,J
)− 1
4(HA[CHD]B + 3ηA[C ηD]B )P1
AB,IP1CD,J
• Lorentz anomaly coefficients
L00IJ = 0
L01IJ = ηABS01AB,IJ −12
ηA[C ηD]B (Q0AB,IP1
CD,J + P1AB,IQ0
CD,J)
L11IJ = ηABS11AB,IJ −12(HA[C ηD]B + ηA[CHD]B )P1
AB,IP1CD,J
− 12
ηA[C ηD]B (Q1AB,IP1
CD,J + P1AB,IQ1
CD,J)
• Basic building blocks:
S11AB,IJ = − 12DADBHIJ −
12(HIKRK
ABJ +HJKRKABI )−HCDΩ C
I AΩ DJ B
− DAHCI Ω CJ B −DAHCJΩ C
I B
S01AB,IJ = RIABJ +12DBGAIJ + ηCDΩ C
I AΩ DJ B +
12(GIDAΩ D
J B −GJDAΩ DI B )
Q1AB,I = −2Ω C
I AHCB − 2DAHBI
Q0AB,I = − 1
2GIAB + Ω C
I AηCB
P1AB,I =
12GIAB + Ω C
I AηCB
Specialize to twisted doubled tori
I Use general flux GABC = λTABCI Lorentz anomaly (TABC = T D
AB HDC ,TABI = T CAB HCDED
I )
L01IJ =
λ2 − 14TIABT AB
J
L11IJ = − (λ− 1)2
4TI ABT
ABJ − λ− 1
4(TI ABT
ABJ + TJABT
ABI )
• Vanish for all gaugings when λ = 1• Compact gaugings
L11IJ = −λ2 − 1
4TIABT
ABJ ,
• Vanish for λ = ±1 as well• Classical Lorentz invariance, once established, survives inthe quantum theory
I Weyl anomaly
W 00IJ =
(λ− 1)2
16(TIABT AB
J − TIABT ABJ )
W 01IJ =
λ− 14
(TIABT AB
J − TIABT ABJ + (λ + 1)TIABT AB
J
)W 11
IJ =(λ + 1) (8− 3(λ + 1))
16TIABT AB
J +(λ + 1) (8− (λ + 1))− 16
16TIABT AB
J
− 14(TIABT
ABJ − TIABT
ABJ )− λ− 1
4(TIABT
ABJ + TJABT
ABI )
• General gaugings with λ = 1: W 00IJ = W 01
IJ = 0• Condition for (one-loop) conformal invariance
W 11AB =
14(ηAE ηBE ′ −HAEHBE ′ )(η
CC ′ηDD ′ −HCC ′HDD ′ )T ECD T E ′
C ′D ′ = 0
• Compact gaugings: W 00IJ = W 01
IJ = 0 for λ = ±1 and
W 11IJ = −λ2 − 1
4TIABT AB
J
• Conformal models for λ = ±1
Correspondence with N = 4 electric gaugings
I Introduce projectors (recall η = Hη−1H)
PABCD± (H) =
12(ηA(CηD)B ±HA(CHD)B)
• Define
ZAB(H) =12(ηC [C ′ηD ′]D −HC [C ′HD ′]D)TCDATC ′D ′B
• Weyl anomaly
WAB = P CD−AB (H)ZCD(H)
• N = 4 gauged supergravity potential (electric gaugings)
V (M) =12
(13MAA′MBB ′MCC ′ +
(23
ηAA′ −MAA′)
ηBB ′ηCC ′)TABCTA′B ′C ′
• Incorporate constraint MAB ∈ O(d ,d)O(d)×O(d)
V = V + Λ BA (MACηCB − ηACMCB)
• Condition for extremum: set to zero
∂V∂MAB = −ZAB(M) +
12(ηACηBD +MABMCD)ΛCD
= −ZAB(M) + P+ABCD(M)ΛCD
• Identify HAB = MAB and act with P−(H)
PABCD− (H)ZCD(H) = 0
• N = 4 electric vacuum ⇒ conformal chiral boson model
I Assume now conformal invariance condition is satisfied. Then
ZAB(H) = P+ABCD(H)ZCD(H)
• Thus
∂V∂MAB
∣∣∣∣M=H
= P+ABCD(H)(
ΛCD − ZCD(H))
• N = 4 vacuum for ΛCD = ZCD(H)
I N = 4 electric vacua ⇔ conformal chiral boson modelsI SUSY: TDT is even-dim group manifold ⇒ N = 2 SCFT
Compact gaugings and chiral WZW models
I Compact gaugings ⇒ conformal chiral boson modelsI Compact gauging conditions for HAB = δAB
habc = Q bca , Rabc = τ a
bc , τ cab = −τ b
ac , Q abc = −Q cb
a
• Change basis Za,X a to T±a = 12 (Za ± X a)
• Gauge algebra is a sum
[T±a ,T±b ] = f ±cab T±c , [T+a ,T−b ] = 0
f ±cab = τ cab ±Q bc
a
• Gauge group GL × GR ∈ O(d)×O(d)
I Corresponding chiral boson model (chiral basis y iL,R = y i ± y i )
S =14
∫d2σ
((GL
ij + λBLij )∂−y
iL∂1y
jL − (GR
ij + λBRij )∂+y
iR∂1y
jR
)• GL,R
IJ and dBL,R invariant metric and 3-form of GL,R• Chiral and antichiral WZW based on GL and GR
[Sonnenscheim ’88; Tseytlin ’91]
• Kac–Moody symmetry ⇒ all order conformal invariance!• When GL = GR : ordinary WZW model• In line with previous observations for GL = GR = SU(2)
[Dabholkar, Hull 05; Dall’Agata, Prezas ’08]
• WZW model is realized in terms of non-geometric fluxes• Notion of non-geometricity needs refinement
Motivation and overview
Fluxes, twists and supergravity gaugings
Non-geometric backgrounds and twisted doubled tori
Interacting chiral boson models: Lorentz invariance
Interacting chiral boson models: one-loop effective action
Summary and open problems
Summary
I Supergravity gaugings: non-geometric string backgrounds• Embedding tensor ⇒ gauge algebra ⇒ all fluxes!• New interpretation: geometric flux on doubled torus• Twisted doubled tori: underlying geometriesI Interacting chiral bosons: doubled geometry sigma models• Twisted doubled tori ⇒ Lorentz invariant chiral bosons• Conformal invariance condition ⇔ Vacua of N = 4 potential• Compact gaugings are always conformal: chiral WZW modelsI Twisted doubled tori are actual physical backgroundsI Scherk–Schwarz on doubled geometries → general
supergravity gaugings
Open problems
I Straightforward generalizations• Include dilaton (gaugings with SO(1, 1) duality twist)• Include non-compact spacetime dimensions• Include worldsheet supersymmetry• Full equations of motion of N = 4 gauged supergravityI Other classes of Lorentz invariant chiral boson models ?I Conformal field theory aspects• Origin of conformal invariance condition• Deformations of (chiral, gauged) WZW models ?
[Tseytlin ’93]
• Relation to affine Virasoro constructions
I Relation to other worldsheet models[Albertsson, Kimura, Reid-Edwards ’08; Hull, Reid-Edwards ’09; Reid-Edwards ’09; Halmagyi ’09]
• Non-commutativity of Q-flux and non-associativity of R-flux ?[Mathai, Rosenberg ’04; Bouwknegt, Hannabuss, Mathai ’04; Ellwood, Hashimoto ’06]
I Connection with double field theory[Hohm, Hull, Zwiebach ’10]
• Equations of motion: beta functionals• Explicit Scherk–Schwarz on twisted doubled torus: electricN = 4 gaugings
I Exotic constructions• Incorporate SL(2,Z) S-duality, double the doubled torus!• Account for all N = 4 gaugings• E7 invariant membrane theory!• Account for all N = 8 gaugings